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A mathematical formulation of accelerating moment release based on the stress accumulation model
A. Mignan, G. C. P. King, D. Bowman

A mathematical formulation of accelerating moment release based on the stress accumulation model

Author / Organization:
Science & Mathematics Published 2007 Verification Pending

Overview & Synopsis

Large earthquakes can be preceded by a period of accelerating seismic activity of moderate-sized earthquakes. This phenomenon, usually termed accelerating moment release, has yet to be clearly understood. A new mathematical formulation of accelerating moment release is obtained from simple stress transfer considerations, following the recently proposed stress accumulation model. This model, based on the concept of elastic rebound, simulates accelerating seismicity from theoretical stress changes during an idealized seismic cycle. In this view, accelerating moment release is simply the consequence of the decrease, due to loading, of the size of a stress shadow due to a previous earthquake. We show that a power law time-to-failure equation can be expressed as a function of the loading rate on the fault that is going to rupture. We also show that the m value, which is the power law exponent, can be defined as m = D/3, with D a parameter that takes into account the geometrical shape of the stress lobes and the distribution of active faults. In the stress accumulation model, the power law is not due to critical processes.

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Document Information

Document Title A mathematical formulation of accelerating moment release based on the stress accumulation model
Author / Organization A. Mignan, G. C. P. King, D. Bowman
Subject & Discipline Multidisciplinary Academic Open Research
Categories Science & Mathematics
Publication Year 2007
License / Rights Open Access / Creative Commons
Resource Verification Listed PDF (Verification Pending)
Original Host Website HAL Open Science (hal.science)
File Format application/pdf (Portable Document Format)
Language EN
Catalog ID DOC-53806
Original Source Link Visit Source Page on hal.science »